Accelerating black hole in 2+1 dimensions and 3+1 black (st)ring

M. Banados, M. Henneaux, C. Teitelboim and J. Zanelli, “Geometry of the (2+1) black hole,” Phys. Rev. D 48

1993

Earlier work this paper cites.

A. R. Steif,“Time-Symmetric Initial Data for Multi-Body Solutions in Three Dimensions,” Phys. Rev. D 53

1996

Earlier work this paper cites.

C. Martinez, C. Teitelboim and J. Zanelli, “Charged rotating black hole in three spacetime dimensions,” Phys. Rev. D 61

2000

Earlier work this paper cites.

D. Ida, “No black hole theorem in three-dimensional gravity,” Phys. Rev. Lett. 85

2000

Earlier work this paper cites.

R. Emparan, G. T. Horowitz and R. C. Myers, “Exact description of black holes on branes. II: Comparison with BTZ black holes and black strings,” JHEP 0001

2000

Earlier work this paper cites.

J. Podolsky and J. B. Griffiths, “Uniformly accelerating black holes in a de Sitter universe,” Phys. Rev. D 63

2002

Cited alongside, same era.

R. Emparan and H. S. Reall, “Generalized Weyl solutions,” Phys. Rev. D 65

2002

Cited alongside, same era.

R. Emparan and H. S. Reall, “A rotating black ring in five dimensions,” Phys. Rev. Lett. 88

2002

Cited alongside, same era.

O. J. C. Dias and J. P. S. Lemos, “Pair of accelerated black holes in anti-de Sitter background: The AdS C-metric,” Phys. Rev. D 67

2003

Cited alongside, same era.

S. Deser and B. Tekin, “Energy in generic higher curvature gravity theories,” Phys. Rev. D 67

2003

Cited alongside, same era.

J. B. Griffiths, P. Krtous and J. Podolsky, “Interpreting the C-metric,” Class. Quant. Grav. 23

2006

Later among the works it cites.

R. Emparan and H. S. Reall, “Black Holes in Higher Dimensions,” Living Rev. Rel. 11

Original

2008

Later among the works it cites.

M. M. Anber, “AdS4/CFT3+Gravity for Accelerating Conical Singularities,” JHEP 0811

Original

2008

Later among the works it cites.

O. Miskovic and J. Zanelli, “On the negative spectrum of the 2+1 black hole,” Phys. Rev. D 79

Original

2009

Later among the works it cites.